1. 1 LIGO-G1100439-v3 Transmission Monitoring Telescope and Suspension – TMS Eric Gustafson aLIGO NSF Review LIGO Livingston Observatory April 25-27, 2011 Auxiliary Optical Systems - AOS

2. Auxiliary Optical System Talks Outline Transmission Monitoring Telescope and Suspension (TMS) – Eric Gustafson Optical Levers (OptLev) – Eric James Thermal Compensation System (TCS) – Phil Willems Initial Alignment System (IAS) – Doug Cook Photon Calibration System (PhotonCal) – Rick Savage Stray Light Control (SLC) and Viewports (VP) – Mike Smith 2 LIGO-G1100439-v3

3. 3 Transmission Monitoring Telescope and Suspension - TMS TMS LIGO-G1100439-v3

4. TMS Functions Collects 1064 nm light transmitting through ETM and provides it for Interferometer Sensing and Control Transmits 532 nm light for Arm Length Stabilization Transmits 532 nm for intermittent Hartmann ETM monitoring Transmit any residual 1064 nm radiation to beam dump 4 LIGO-G1100439-v3

5. 5 TMS Requirements Suspension and Noise »6 DOF of platform are isolated »Suspension Eigen frequencies between 0.5-5 Hz »All rigid body modes damped to Q<10 »Above 10 Hz isolation factor > 1000 all 6 DOF –Displacement noise < 1 pm/ √ (Hz)] –Angular noise < 1 frad/ √ (Hz)] »Internal modes of suspension structure 150 Hz or higher »At 3 Hz isolation factor >10 all DOF Telescope »Reduce 1064 nm beam by 20x to fit 2 inch optics on optics table »Alignment sensors with 90 degree Gouy phases within ± 10 deg. »Handle 1064 nm, 532 nm sensor wavelengths LIGO-G1100439-v3

6. TMS Design Concept Double pendulum suspension based on upper stage of Quad Suspension Telescope »Reflective off-axis parabolic mirrors »Folded design Optical routing done on optical table High Power in vacuum beam dump 6 LIGO-G1100439-v3

7. TMS Development Accomplishments Compared Three Telescope Designs and selected off axis parabolic design Telescope modeled with Ray Tracing Program Modeled Suspension Transfer Functions with LIGO Software 7 LIGO-G1100439-v3

8. 8 TMS Suspension Prototype Tests Establish all 6 BOSEMs operational and interference free Measured all 12 body resonance frequencies Response Rough cut at orthogonalizing DOF response Confirm resonant frequencies assignments via TF for all DOFs Good agreement with prototype model Established good damping Typical broadband noise excitation TF (nominal Roll drive) Roll resonanc es Roll (red) sensed LIGO-G1100439-v3

9. TMS Telescope Mirror Alignment & Characterization Shack-Hartmann Test Facility @ Caltech Incoming inspection of parabolic mirrors Wave front distortion spec. <1/20λ @ 1064nm 9 LIGO-G1100439-v3 Zernike Polynomial Coefficient Off-axis Parabolic Mirror Incoming Inspection

10. TMS Telescope Mirror Alignment & Characterization Alignment with Shack-Hartmann sensor leaves mainly a defocus component in the Zernike’s polynomial with no astigmatism => telescope meets the astigmatism specification 10 LIGO-G1100439-v3 Zernike Polynomial Coefficient Z 4 = -0.030 Z 6 = 0.036 Z 4 = -0.001 Z 6 = 0.000 Astigmatism Correction

11. TMS Development Plan Preliminary Design Review completed - May 2010 ✔ Telescope First Article build – May 2011 Final Design Phase »Optical Table tests completed – April 2011 ✔ »Telescope First Article tests completed – June 2011 »Suspension testing completed – March 2011 ✔ »FDR completed – June 2011 »Update all drawings – June 2011 11 LIGO-G1100439-v3

12. TMS Project Organization and Plans Project Organization »Team Leader/Mechanical Engineer - Ken Mailand - Caltech »Cognizant Scientist - Sam Waldman – MIT »Telescope Optical Design – Mike Smith - Caltech »Mechanical Designer – Mike Miller– Caltech »Draftsperson - Jesse Terraza – Caltech »Electronics – Jay Heefner – Caltech »Suspensions Modeling - Matt Evans - MIT »Suspensions Testing – Bill Kells - Caltech »Optical Testing - Virginio Sannibale – Caltech »Assembly Technician – Larry Mossberger - Caltech »Project Engineer and Planning – Lisa Austin - Caltech Project Plans »Reworked First Article available for Long Arm Test – June 2011 »Remaining production units available – December 2011 12 LIGO-G1100439-v3

13. TMS Challenges, Risks, and Mitigations Getting First Article delivered to Hanford in time for the Long Arm Test »Draftsperson »Assembly Technician »Project Engineer and Planning Optical Aligning and focusing double off axis parabolic telescope »Course alignment with auto collimating telescope »Fine alignment with Shack-Hartmann sensor »Simulation of final alignment with ray tracing simulation »Incoming testing of all parabolic mirrors Delivery of off-axis parabolic mirrors »Two suppliers »First Article already Received August 2010 and second Due April 2011 13 LIGO-G1100439-v3

14. TMS Near Term Activities Build and Test First Article Telescope – June 2011 Design and procure the equipment needed for testing »Suspension test stand – Caltech – May 2011 »Electronics test stand – Caltech Completed ✔ »Fixturing for Telescope testing – Caltech – May 2011 Final Design Review – June 2011 Rework First Article Telescope in time for Long Arm Test 14 LIGO-G1100439-v3